Abstract
The importance of temperature is very often not fully recognized, the reason probably being that our life is restricted to an extremely narrow range of temperatures. This can be realized if we look at the temperatures existing in nature or accessible in laboratories (Fig.1.1). These temperatures range from about 109 K, the temperature at the centre of the hottest stars and necessary to form or destroy atomic nuclei, to about 10−5 K, the lowest temperatures accessible today in the laboratory in condensed matter physics experiments. This lower limit means that we have been able to refrigerate matter to within about 10 µK of absolute zero (0K = −273.15° C).
Keywords
- Absolute Zero
- Magnetic Refrigeration
- Thermal Boundary Resistance
- Adiabatic Demagnetization
- Millikelvin Temperature
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© 1992 Springer-Verlag Berlin Heidelberg
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Pobell, F. (1992). Introduction. In: Matter and Methods at Low Temperatures. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-08578-3_1
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DOI: https://doi.org/10.1007/978-3-662-08578-3_1
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